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Mineralogy and Physicochemical Features of Saharan Dust Wet Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2018-211 Manuscript under review for journal Atmos. Chem. Phys. Discussion started: 1 March 2018 c Author(s) 2018. CC BY 4.0 License. Mineralogy and physicochemical features of Saharan dust wet deposited in the Iberian Peninsula during an extreme red rain event Carlos Rodriguez-Navarro, Fulvio di Lorenzo, and Kerstin Elert Dept. Mineralogy and Petrology, University of Granada, Fuentenueva s/n, 18002 Granada, Spain 5 Correspondence to: Carlos Rodriguez-Navarro ([email protected]) Abstract. The mineralogy and physicochemical features of Saharan dust particles help to identify source areas and determine their biogeochemical, radiative and health effects, but their characterization is challenging. Using a multianalytical approach, here we characterized with unprecedented level of detail the mineralogy and physicochemical properties of Saharan dust particles massively wet deposited (~18 g m-2) following an extreme "red rain" event triggered by a north 10 African cyclone that affected the southern Iberian Peninsula during February 21-23, 2017. Abundant palygorskite and illite, and relatively high carbonate contents, well-known northern and north-western Saharan dust indicators, along with low chlorite content and significant amounts of smectites and kaolinite, whose abundance increases southwards in the western Sahara, complemented by satellite imagery and back/forward trajectories, show that the most probable dust source areas were (i) south/central Algeria, north Mali and northwest Niger, and (ii) north Algeria, south Tunisia and north-west Libia. 15 Scanning and transmission electron microscopy analyses, including Z-contrast high angle annular dark field (HAADF) imaging and analytical electron microscopy (AEM) show that clay minerals include abundant structural Fe (57 % of the total Fe) and typically form nanogranular aggregates covered or interspersed with amorphous/poorly crystalline iron oxyhydroxide nanoparticles (ferrihydrite), which account for 28 % of the free Fe, the rest being goethite and hematite. These nanogranular aggregates tend to form rims lining large silicate and carbonate particles. Such internally mixed iron-containing 20 phases are main contributors to the observed absorption of solar and thermal radiation, and along with the abundant coarse/giant particles (>10 μm), strongly affect the dust direct radiative forcing. The lack of secondary sulfates in aggregates of unaltered calcite internally mixed with clays/iron-rich nanoparticles shows that iron-rich nanoparticles did not form via atmospheric (acid) processing but were already present in the dust source soils. Such iron-rich nanoparticles, in addition to iron-containing clay (nano)particles, are an important source for bioavailable (soluble) iron. The dust particles are a potential 25 health hazard, specially the abundant and potentially carcinogenic iron-containing palygorskite fibers. Ultimately, we show that different source areas are activated over large desert extensions, and large quantities of complex dust mixtures are transported thousands of kilometers and wet-deposited during such extreme events, which thwart any other Saharan dust event affecting south-western Europe. The past, present, and future trends, as well as impacts, of such extreme events must be taken into account when evaluating and modeling the manifold effects of the desert dust cycle. 1 Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2018-211 Manuscript under review for journal Atmos. Chem. Phys. Discussion started: 1 March 2018 c Author(s) 2018. CC BY 4.0 License. 1 Introduction Aeolian erosion of semi-arid and arid desert surfaces contributes to an estimated ~ 1,000 to 3,000 Tg yr−1 global emission of mineral dust aerosol (Goudie and Middleton, 2001; Engelstaedter et al., 2006; Cakmur et al., 2006). The impact of desert dust is enormous (Gieré and Querol, 2010): (i) it directly affects atmospheric radiative balance due to scattering and 5 absorption of solar and terrestrial radiation, thereby affecting atmospheric dynamics and climate (Carlson and Benjamin, 1980; Tegen and Lacis 1996: Ramanathan et al., 2001; Tegen, 2003; Balkanski et al., 2007). Indirectly, it also affects climate via its potential for altering atmospheric physics/microphysics (i.e., acting as nuclei for liquid and solid cloud droplets) and the hydrological cycle (Ramanathan et al., 2001). Such direct and indirect forcings strongly depend on mineral dust physicochemical properties, including particle size, shape and composition/mineralogy (Tegen, 2003; Lafon et al., 2006; 10 Formenti et al., 2011; Mahowald et al., 2014; Zhang et al., 2015; Kok et al., 2017); (ii) it supplies sediments to downwind marine and continental areas, affecting the surface albedo of the later, whereas dust entrainment in source regions is a major erosive agent, strongly affecting soil quality (Goudie and Middleton, 2001); (iii) it also supplies key micronutrients (e.g., iron and phosphorous) to distal ocean and inland water environments, directly affecting the C cycle via stimulated bioproductivity, and indirectly affecting climate via atmospheric CO2 sequestration (Jickells et al., 2005; Raiswell and 15 Canfield, 2012); (iv) it is involved in a range of heterogeneous reactions with manifold implications (Usher et al., 2003). For instance, carbonates in Saharan dust increase the pH of precipitation acting as a buffer for acid rain in Europe (Loÿe-Pilot et al., 1986); (v) desert dust storms are a hazard with detrimental effects on transportation (e.g., reduced visibility), infrastructure, and (solar) energy generation (Middleton, 2017), also causing soiling and discoloration of monuments (Comite et al., 2017); (vi) desert mineral dust is a health hazard to humans (Karanasiou et al., 2012; Goudie, 2014). Exposure 20 to desert dust (particulate matter with size < 10 µm, PM10 and/or with size < 2.5 µm, PM2.5) has been associated with morbidity and premature death due to dust-related (or enhanced) cardiovascular and respiratory problems (Perez et al., 2008), as well as several diseases related to dust-borne microorganisms (short-term effects) (Griffin, 2007). In addition, silicosis/pulmonary fibrosis (desert lung) and cancer-related illnesses have been associated with desert dust exposure (long term effects) (Giannadaki et al., 2014). 25 More than half of the global mineral dust aerosol comes from northern Africa (Sahara/Sahel) (Goudie and Middleton, 2001; Prospero et al., 2002; Engelstaedter et al., 2006), with an estimated ~700−1600 Tg of Saharan dust exported yearly across the Mediterranean sea to Europe and the near-East, the Red sea to the near-East and Asia, and the North Atlantic ocean to the Americas (D'Almeida, 1986; Prospero, 1996; Goudíe and Middleton, 2001). Although most Saharan dust is transported across the Atlantic Ocean (Carlson and Prospero, 1972), an estimated 80–120 Tg yr-1 is 30 transported northward across the Mediterranean sea to Europe (D'Almeida, 1986). It has been pointed out that the strength of the Saharan dust input increased since ca. mid 20th century due to recurrent droughts in North Africa (Prospero and Lamb, 2003), anthropogenic-induced desertification (Moulin and Chiapello, 2006), changes in land use, including an increase in cultivable lands in the Sahel region (Mulitza et al., 2010), and other larger-scale phenomena (e.g., atmospheric circulation 2 Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2018-211 Manuscript under review for journal Atmos. Chem. Phys. Discussion started: 1 March 2018 c Author(s) 2018. CC BY 4.0 License. patterns and/or climate change) (Sala et al., 1996; Moulin et al., 1997). Nonetheless, there is evidence for significant seasonal to decadal variability of Saharan dust strength. Indeed, since the end of the 1980s, a trend towards decreasing Saharan dust across the tropical North Atlantic has been reported (Ridley et al., 2014; Evans et al. 2016). In contrast, the strength of Saharan dust affecting southern Europe has reportedly increased in recent decades (Antoine and Nobileau, 2006), 5 with dust plume intrusions being currently rather common (Escudero et al., 2005; Avila et al., 2007; Titos et al., 2017). They lead to both dry and wet deposition of mineral dust (Escudero et al., 2005). Wet deposition typically occurs as "red rain", "dust rain", "blood rain" or "muddy rain", events that periodically and persistently affect southern Europe (Prodi and Fea, 1979), and most particularly the Iberian Peninsula (Sala et al., 1996; Avila et al., 1997; White et al., 2012), the European region closest to North Africa. Although known since ancient times (Gieré and Querol, 2010), red rain events have 10 experienced a remarkable increase in their frequency and intensity over the last decades (Sala et al., 1996; Escudero et al., 2005; Fiol et al., 2005; Avila et al., 2007). In some cases they are extreme, with 10−40 g m-2 of dust deposited after a single red rain event (Avila et al., 1997; 2007; Fiol et al., 2005), thwarting the average yearly Saharan dust deposition in south- western Europe, estimated to be about 3−14 g m-2 (Goudie and Middleton, 2001). This was the case of the last extreme red rain event that took place in the area of Granada (south of Spain) in February 21st−23rd, 2017. 15 The global significance and impact of desert-derived mineral dust aerosol has attracted extensive research focused on analyzing dust composition, mineralogy, physical properties, sources, and entrainment-transport-deposition mechanisms
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